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Relevant bibliographies by topics / Astrophysics and Cosmology

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Academic literature on the topic 'Astrophysics and Cosmology'

Author: Grafiati

Published: 4 June 2021

Last updated: 1 February 2022

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Journal articles on the topic "Astrophysics and Cosmology"

1

Tavakol, R. K. "Fragility in Cosmology and Astrophysics." International Astronomical Union Colloquium 132 (1993): 399–405. http://dx.doi.org/10.1017/s025292110006629x.

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AbstractThe theoretical framework adopted in astrophysics and cosmology, in both modelling and the analysis of the observational data, is often implicitly assumed to be that of structural stability. Here, in view of some of the recent results in dynamical systems theory, it is argued that such a framework cannot be assumed a priori and that the fragility framework may instead turn out to be the appropriate framework for the study of certain phenomena in the astrophysical and the cosmological settings. This is motivated by a number of examples from cosmology and a brief discussion of some of the potential domains of its relevance in astrophysics.

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Colafrancesco, Sergio. "Multi-Frequency Study of the SZ Effect in Cosmic Structures." Acta Polytechnica CTU Proceedings 1, no. 1 (December 4, 2014): 56–65. http://dx.doi.org/10.14311/app.2014.01.0056.

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The Sunyaev-Zel’dovich effect (SZE) is a relevant probe for cosmology and astrophysics. A multi-frequency approach to study the SZE in cosmic structures turns out to be crucial in the use of this probe for astrophysics and cosmology. Astrophysical and cosmological applications to galaxy clusters, galaxies, radiogalaxies and large-scale structures are discussed. Future directions for the study of the SZE and its polarization are finally outlined.

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Colafrancesco, Sergio. "THE SZ EFFECT IN THE PLANCK ERA: ASTROPHYSICAL AND COSMOLOGICAL IMPACT." Acta Polytechnica 53, A (December 18, 2013): 560–72. http://dx.doi.org/10.14311/ap.2013.53.0560.

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The Sunyaev–Zel’dovich effect (SZE) is a relevant probe for cosmology and particle astrophysics. The Planck Era marks a definite step forward in the use of this probe for astrophysics and cosmology. Astrophysical applications to galaxy clusters, galaxies, radiogalaxies and large-scale structures are discussed. Cosmological relevance for the Dark Energy equation of state, modified Gravity scenarios, Dark Matter search, cosmic magnetism and other cosmological applications is also reviewed. Future directions for the study of the SZE and its polarization are finally outlined.

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Bergström, Lars, Ariel Goobar, and Andrew H. Jaffe. "Cosmology and Particle Astrophysics." American Journal of Physics 69, no. 3 (March 2001): 394. http://dx.doi.org/10.1119/1.1336841.

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Bergström, Lars, Ariel Goobar, and Andreas J. Albrecht. "Cosmology and Particle Astrophysics." Physics Today 53, no. 3 (March 2000): 73–74. http://dx.doi.org/10.1063/1.883006.

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Auriemma, Giulio. "LHC, Astrophysics and Cosmology." Acta Polytechnica CTU Proceedings 1, no. 1 (December 4, 2014): 42–48. http://dx.doi.org/10.14311/app.2014.01.0042.

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In this paper we discuss the impact on cosmology of recent results obtained by the LHC (Large Hadron Collider) experiments in the 2011-2012 runs, respectively at √<span style="text-decoration: overline;">s</span> = 7 and 8 TeV. The capital achievement of LHC in this period has been the discovery of a spin-0 particle with mass 126 GeV/c<sup>2</sup>, very similar to the Higgs boson of the Standard Model of Particle Physics. Less exciting, but not less important, negative results of searches for Supersymmetric particles or other exotica in direct production or rare decays are discussed in connection with particles and V.H.E. astronomy searches for Dark Matter.

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BINÉTRUY, P. "PARTICLE ASTROPHYSICS AND COSMOLOGY." International Journal of Modern Physics A 20, no. 22 (September 10, 2005): 5193–201. http://dx.doi.org/10.1142/s0217751x05028703.

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Szalay, Alexander, John Peacock, Y. Chu L. da Costa, J. Einasto, G. Ellis, D. Koo, S. Lilly, et al. "Commission 47: Cosmology: (Cosmologie)." Transactions of the International Astronomical Union 24, no. 1 (2000): 311–14. http://dx.doi.org/10.1017/s0251107x00003242.

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Cosmology is one of the most dynamically evolving areas of astrophysics today. Twenty years ago the estimates of the amplitude of the primordial fluctuations were about 10-3, almost a factor of 100 off of today’s measurements. Ten years ago we could only hope for high precision measurements of large scale structure, there were less than 5000 redshifts measured, and only a handful of normal galaxies with z > 1 were known. Computer models of structure formation had just begun to consider non-power-law spectra based on physical models like hot/cold dark matter. As a consequence there was considerable freedom in adjusting parameters in the various galaxy formation scenarios. In contrast, many of today’s debates are about factors of 2 and soon we will be arguing about 10% differences. The Harrison-Zeldovich shape of the primordial fluctuation spectrum, first derived from philosophical arguments can now be quantified from detections of fluctuations by COBE. The number of available redshifts is beyond 50,000, and soon we will have redshift surveys surpassing 1 million galaxies. N-body simulations are becoming more sophisticated, of higher resolution, and incorporating complex gas dynamics.

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HENLEY, ERNEST M. "NEUTRINO ASTROPHYSICS." Modern Physics Letters A 19, no. 13n16 (May 30, 2004): 1145–53. http://dx.doi.org/10.1142/s0217732304014495.

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Netchitailo, Vladimir S. "Dark Matter Cosmology and Astrophysics." Journal of High Energy Physics, Gravitation and Cosmology 05, no. 04 (2019): 999–1050. http://dx.doi.org/10.4236/jhepgc.2019.54056.

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Dissertations / Theses on the topic "Astrophysics and Cosmology"

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Whiting, Alan B. "Local cosmology." Thesis, University of Cambridge, 1997. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.360010.

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Wong, D. "Cosmology and superstrings." Thesis, University of Sussex, 1987. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.381634.

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Webster, R. L. "Gravitational lensing and cosmology." Thesis, University of Cambridge, 1985. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.355284.

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Nilsson, Ulf. "Dynamical systems in cosmology and astrophysics /Ulf Nilsson." Stockholm : Stockholms Universitet, 1998. http://www.gbv.de/dms/goettingen/254604390.pdf.

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Keränen, Petteri. "Aspects of massive neutrinos in astrophysics and cosmology." Helsinki : University of Helsinki, 1999. http://ethesis.helsinki.fi/julkaisut/mat/fysii/vk/keranen/.

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Powell, Andrew James. "The cosmology and astrophysics of axion-like particles." Thesis, University of Oxford, 2016. https://ora.ox.ac.uk/objects/uuid:bbbb3cbc-a0ba-4024-86b0-c720d8104270.

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In this thesis I study astrophysical and cosmological effects of axion-like particles (ALPs). ALPs are pseudo-scalar particles, which are generally very weakly-interacting, with a coupling α/M E · B to electromagnetism. They are predicted by many theories which extend the standard model (SM) of particle physics, most notably string theory. String theory compactifications also predict many scalar fields called moduli which describe the size and shape of the extra, compact dimensions. In string theory models generically the moduli fields are responsible for reheating the universe after inflation. Being gravitationally-coupled, they will also decay to any other particles or sectors of the theory, including any light ALPs, of which there are usually many. The ALPs produced by moduli decay will contribute to dark radiation, additional relativistic energy density. The amount of dark radiation is tightly constrained by observations, this bounds the branching fraction of moduli decays into ALPs, which constrains the string theory model itself. I calculate the amount of dark radiation produced in a model with one light modulus, solely responsible for reheating, called the Large Volume Scenario. I study a minimal version of this model with one ALP and a visible sector comprised of the minimal supersymmetric SM. The dominant visible sector decay mode is to two Higgses, I include radiative corrections to this decay and find that ALP dark radiation is over-produced in this minimal version of the model, effectively ruling it out. The production of ALPs from moduli decay at reheating seems to be a generic feature of string theory models. These ALPs would exist today as a homogeneous cosmic ALP background (CAB). The coupling of ALPs to electromagnetism allows ALPs to convert to photons and vice versa in a magnetic field, leading to potential observable astrophysical signals of this CAB. Observations have shown an excess in soft X-ray emission from many galaxy clusters. I use detailed simulations of galaxy cluster magnetic fields to show that a CAB can explain these observations by conversion of ALPs into X-ray photons. I simulate ALP-photon conversion in four galaxy clusters and compare to soft X-ray observations. I show the excesses (or lack thereof) can be fit consistently across the clusters for a CAB with ALP-photon inverse coupling of M = 6 - 12 x 10¹² GeV, if the CAB spectrum has energy ~ 200 eV. I also study the possibility of using galaxy clusters to search for and constrain the ALP coupling to photons using cluster X-ray emission. Conversion of X-ray photons into ALPs will cause spectral distortions to the thermal X-ray spectrum emitted by galaxy clusters. I show that the non-observation of these distortions is able to produce the strongest constraints to date on the ALP-photon inverse coupling, M ≳ 7 x 10¹¹ GeV.

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Mellor, Felicity Avril. "Black holes and quantum cosmology." Thesis, University of Newcastle Upon Tyne, 1990. http://hdl.handle.net/10443/682.

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The work of this thesis falls into two parts: a discussion of decoherence in quantum Kaluza-Klein theories and a study of some of the properties of general black hole metrics in de Sitter spacetime. Kaluza-Klein theories permit a variety of compactifications and arbitrary scales for the internal space. There must be no quantum interference between these different possibilities. In chapter one it is demonstrated that in the Salam-Sezgin compactification interference between differently scaled interenal spaces is suppressed. In chapter two new gravitational instantons are presented which are related to charged, rotating black holes with a cosmological constant A. These instantons correspond to black holes in de Sitter space with identical Hawking temperatures. Their action contributes terms of order A-1/2 to path integrals with quantum wormholes. The metrics of these general de Sitter black holes show that the spacetimes have wormholes connecting different asymptotic regions. In chapter three the theory of black hole perturbations is extended to these metrics. It appears that the holes are stable even at the Cauchy horizon. This implies that cosmic censorship is violated. The stability of the spacetimes also implies the existence of a cosmological no hair theorem.

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Stevenson, Paul Robert Frederick. "Faint galaxy photometry and cosmology." Thesis, Durham University, 1985. http://etheses.dur.ac.uk/6800/.

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Deep galaxy catalogues have been constructed from automatic measurements of photographic plates by the COSMOS machine at the Royal Observatory Edinburgh. The plates were taken by the 1.2m UK Schmidt telescope (UKST) and 4m Anglo-Australian telescope (AAT), in both blue and red passbands. The UKST plates cover an area of sky of~170 square degrees, some four times larger than any previous study to these depths (B-21, R~20mag).By comparing the UKST and AAT galaxy number-magnitude counts and colour distributions with those predicted using computer models, evidence for luminosity evolution has been obtained. The red passband counts require less luminosity evolution than in the blue passband and at the faintest magnitudes reached here (R'-22mag) the cosmological parameter, q(_o), has as large an effect. The red count models are well enough determined to reject world models with q(_o)> 1. In order to further separate the effects of luminosity evolution and q^, the possibility of using a well determined Hubble diagram or faint "galaxy redshift surveys is considered. The galaxy two-point angular correlation function, w(ɵ), has been estimated from the UKST catalogues and shows evidence of a feature at large angular scales, corresponding to a spatial separation of ~3h Mpc (H(_o) = l00h kms Mpc ). In a study of the correlation function scaling relation it is found that the observed clustering amplitudes at AAT depths are lower than those predicted using well determined models that assume no clustering evolution. However, sampling errors are large and more 4m data is required in order to test the reality of this result. Also discussed is the possibility of discriminating between recent theories of galaxy formation using the w(#) observations. The method of Turner and Gott has been used to automatically detect groups and clusters of galaxies in the UKST catalogues. It is found that the cluster-cluster w(f) is several times higher than the galaxy-galaxy w(4) when scaled to the same depth. The implications of this result for galaxy formation theories are discussed. By using the average magnitude, m, of a cluster as a distance estimator the redshift distribution of the clusters has been obtained. Features present in these distributions^ may correspond to the effects of superclustering on scales < l50h (^-1)Mpc. The modelled m:distance relation has been used to set constraints on the galaxy luminosity function and hence help to more tightly constrain the number count and clustering models. The orientations of galaxies within clusters and the orientations and ellipticity distributions of the clusters themselves have been used in order to obtain further constraints on the theories of galaxy formation.

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Skea, T. "Anisotropic cosmology and curvature invariants." Thesis, University of Sussex, 1986. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.381633.

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Borrill, Julian. "The cosmology of global texture." Thesis, University of Sussex, 1993. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.335012.

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Books on the topic "Astrophysics and Cosmology"

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Muncaster, Roger. Astrophysics and cosmology. Cheltenham: Stanley Thornes, 1997.

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1915-, Shapiro Maurice M., Stanev Todor, and Wefel J. P, eds. Relativistic astrophysics and cosmology. River Edge, NJ: World Scientific, 2004.

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Bergstrom, L. (Lars). Cosmology and particle astrophysics. 2nd ed. United States: PRAXIS PUBLISHING (UK), 2004.

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Shapiro, Maurice M. Particle Astrophysics and Cosmology. Dordrecht: Springer Netherlands, 1993.

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Bergström, L. Cosmology and particle astrophysics. 2nd ed. Berlin: Springer, 2003.

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Peratt, Anthony L., ed. Plasma Astrophysics and Cosmology. Dordrecht: Springer Netherlands, 1995. http://dx.doi.org/10.1007/978-94-011-0405-0.

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Hoyng, Peter. Relativistic Astrophysics and Cosmology. Dordrecht: Springer Netherlands, 2006. http://dx.doi.org/10.1007/978-1-4020-4523-3.

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Shapiro, Maurice M., Rein Silberberg, and John P. Wefel, eds. Particle Astrophysics and Cosmology. Dordrecht: Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1707-4.

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Ariel, Goobar, ed. Cosmology and particle astrophysics. Chichester: Wiley, 1999.

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International School of Cosmic-Ray Astrophysics. Relativistic astrophysics and cosmology. Singapore: World Scientific, 2004.

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Book chapters on the topic "Astrophysics and Cosmology"

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Buchheim, Robert K. "Astrophysics and cosmology." In Astronomical Discoveries You Can Make, Too!, 381–479. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-15660-6_5.

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Trimble, Virginia. "Astrophysics and Cosmology." In AIP Physics Desk Reference, 119–44. New York, NY: Springer New York, 2003. http://dx.doi.org/10.1007/978-1-4757-3805-6_5.

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Glendenning, Norman K. "Cosmology." In Astronomy and Astrophysics Library, 187–207. New York, NY: Springer New York, 2007. http://dx.doi.org/10.1007/978-0-387-47109-9_5.

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Occhionero, F. "Relativistic Astrophysics and Cosmology." In Recent Developments in General Relativity, 447–48. Milano: Springer Milan, 2000. http://dx.doi.org/10.1007/978-88-470-2113-6_38.

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Brandenberger, Robert H., and João Magueijo. "Imaginative Cosmology." In Astrophysics and Space Science Library, 331–71. Dordrecht: Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-011-4175-8_7.

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Coley, A. A. "String Cosmology." In Astrophysics and Space Science Library, 116–39. Dordrecht: Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-0327-7_10.

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Longair, M. S. "Classical Cosmology." In Astrophysics and Space Science Library, 369–79. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-0794-5_37.

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Bond, J. Richard. "Gastrophysical Cosmology." In Astrophysics and Space Science Library, 3–26. Dordrecht: Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-1882-8_1.

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Borgani, Stefano. "Cosmology and Astrophysics with Clusters of Galaxies (Invited)." In Multiwavelength Cosmology, 191–98. Dordrecht: Springer Netherlands, 2004. http://dx.doi.org/10.1007/0-306-48570-2_40.

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Hartle, James B. "Prediction in Quantum Cosmology." In Gravitation in Astrophysics, 329–60. Boston, MA: Springer US, 1987. http://dx.doi.org/10.1007/978-1-4613-1897-2_12.

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Conference papers on the topic "Astrophysics and Cosmology"

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Henneaux, Marc. "Astrophysics and Cosmology." In 26th Solvay Conference on Physics: “Astrophysics and Cosmology”. WORLD SCIENTIFIC, 2016. http://dx.doi.org/10.1142/9789814759182_0001.

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Gottlöber, S., J. P. Mücket, and V. Müller. "Relativistic Astrophysics and Cosmology." In Tenth Seminar. WORLD SCIENTIFIC, 1992. http://dx.doi.org/10.1142/9789814537698.

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Buitrago, J., E. Mediavilla, and A. Oscoz. "Relativistic Astrophysics and Cosmology." In Spanish Relativity Meeting. WORLD SCIENTIFIC, 1997. http://dx.doi.org/10.1142/9789814529525.

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BINÉTRUY, P. "PARTICLE ASTROPHYSICS AND COSMOLOGY." In Proceedings of the 32nd International Conference. World Scientific Publishing Company, 2005. http://dx.doi.org/10.1142/9789812702227_0013.

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Krauss, Lawrence M. "Cosmology and astrophysics 1992." In Proceedings of the XXVI international conference on high energy physics. AIP, 1992. http://dx.doi.org/10.1063/1.43492.

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Balantekin, A. B. "Neutrinos in astrophysics and cosmology." In CETUP* 2015 – WORKSHOP ON DARK MATTER, NEUTRINO PHYSICS AND ASTROPHYSICS AND PPC 2015 – IXTH INTERNATIONAL CONFERENCE ON INTERCONNECTIONS BETWEEN PARTICLE PHYSICS AND COSMOLOGY. Author(s), 2016. http://dx.doi.org/10.1063/1.4953293.

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Abazajian, Kev. "Neutrinos in Astrophysics and Cosmology." In Theoretical Advanced Study Institute 2020 "The Obscure Universe: Neutrinos and Other Dark Matters" - TASI2020. Trieste, Italy: Sissa Medialab, 2021. http://dx.doi.org/10.22323/1.388.0001.

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Vargas, T., Da-Shin Lee, Wolung Lee, and She-Sheng Xue. "Quantum cosmology with nontrivial topologies." In RELATIVISTIC ASTROPHYSICS: 5th Sino-Italian Workshop on Relativistic Astrophysics. AIP, 2008. http://dx.doi.org/10.1063/1.3012282.

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Mather, John C. "Cosmology from the moon." In Astrophysics from the Moon. AIP, 1990. http://dx.doi.org/10.1063/1.39334.

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Wu, Zhong Chao, Da-Shin Lee, Wolung Lee, and She-Sheng Xue. "The Cosmological Constant in Quantum Cosmology." In RELATIVISTIC ASTROPHYSICS: 5th Sino-Italian Workshop on Relativistic Astrophysics. AIP, 2008. http://dx.doi.org/10.1063/1.3012283.

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Reports on the topic "Astrophysics and Cosmology"

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Li, Hui. Astrophysics/Cosmology Status Report. Office of Scientific and Technical Information (OSTI), August 2017. http://dx.doi.org/10.2172/1375895.

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Li, Hui. Strategic Directions for FY18-20: Astrophysics and Cosmology. Office of Scientific and Technical Information (OSTI), August 2017. http://dx.doi.org/10.2172/1375894.

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Wang, Anzhong. Horava-Lifshitz Theory and Applications to Cosmology and Astrophysics. Office of Scientific and Technical Information (OSTI), August 2014. http://dx.doi.org/10.2172/1163093.

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Pulido, Jesus J., Zarija Lukic, Paul Thorman, Caixia Zheng, James Paul Ahrens, and Bernd Hamann. Data Reduction Using Lossy Compression for Cosmology and Astrophysics Workflows. Office of Scientific and Technical Information (OSTI), August 2018. http://dx.doi.org/10.2172/1467236.

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Lyons, L. Proceedings of the Conference on Statistical Problems for Particle Physics, Astrophysics and Cosmology (PHYSTAT2003). Office of Scientific and Technical Information (OSTI), March 2004. http://dx.doi.org/10.2172/826884.

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